The PHASES Differential Astrometry Data Archive. V. Candidate Substellar Companions to Binary Systems

@article{Muterspaugh2010ThePD,
  title={The PHASES Differential Astrometry Data Archive. V. Candidate Substellar Companions to Binary Systems},
  author={Matthew W. Muterspaugh and Benjamin F. Lane and Shrinivas R. Kulkarni and Maciej Konacki and Bernard F. Burke and M. Mark Colavita and Michael Shao and William I. Hartkopf and Alan P. Boss and Monash University and Draper Laboratory and Caltech and Nicolaus Copernicus Astronomical Center Torun and Mit and Jpl and Usno and Carnegie Dtm},
  journal={The Astronomical Journal},
  year={2010},
  volume={140},
  pages={1657-1671}
}
The Palomar High-precision Astrometric Search for Exoplanet Systems monitored 51 subarcsecond binary systems to evaluate whether tertiary companions as small as Jovian planets orbited either the primary or secondary stars, perturbing their otherwise smooth Keplerian motions. Six binaries are presented that show evidence of substellar companions orbiting either the primary or secondary star. Of these six systems, the likelihoods of two of the detected perturbations to represent real objects are… 
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The Phases Differential Astrometry Data Archive. III. Limits to Tertiary Companions
The Palomar High-precision Astrometric Search for Exoplanet Systems (PHASES) monitored 51 subarcsecond binary systems to evaluate whether tertiary companions as small as Jovian planets orbited either
THE PHASES DIFFERENTIAL ASTROMETRY DATA ARCHIVE. II. UPDATED BINARY STAR ORBITS AND A LONG PERIOD ECLIPSING BINARY
Differential astrometry measurements from the Palomar High-precision Astrometric Search for Exoplanet Systems have been combined with lower precision single-aperture measurements covering a much
THE PHASES DIFFERENTIAL ASTROMETRY DATA ARCHIVE. I. MEASUREMENTS AND DESCRIPTION
The Palomar High-precision Astrometric Search for Exoplanet Systems (PHASES) monitored 51 subarcsecond binary systems to determine precision binary orbits, study the geometries of triple and
THE PHASES DIFFERENTIAL ASTROMETRY DATA ARCHIVE. IV. THE TRIPLE STAR SYSTEMS 63 Gem A AND HR 2896
Differential astrometry measurements from the Palomar High-precision Astrometric Search for Exoplanet Systems (PHASES) are used to constrain the astrometric orbit of the previously known ≾2 day
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